Millimetric Sardinia radio Telescope Receiver based on Array of Lumped elements kids
| Autor: | D'Alessandro, G., Barbarava, E., Battistelli, E. S., de Bernardis, P., Cacciotti, F., Capalbo, V., CARRETTI, ETTORE, Columbro, F., Coppolecchia, A., Cruciani, A., De Petris, M., GOVONI, FEDERICA, Isopi, G., Lamagna, L., MARONGIU, Pasqualino, Masi, S., Mele, L., Molinari, M., MURGIA, MATTEO, NAVARRINI, Alessandro, ORLATI, ANDREA, Paiella, A., Pettinari, G., Piacentini, F., PISANU, Tonino, POPPI, Sergio, Presta, G., Radiconi, F. |
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| Jazyk: | angličtina |
| Rok vydání: | 2022 |
| Předmět: |
cluster of galaxies
Astrophysics::High Energy Astrophysical Phenomena Physics QC1-999 Millimetric wavelengths high resolution astrophysics Astrophysics::Instrumentation and Methods for Astrophysics Instrument Millimetric wavelengths high resolution astrophysics cluster of galaxies Instrument Astrophysics::Cosmology and Extragalactic Astrophysics |
| Zdroj: | EPJ Web of Conferences, Vol 257, p 00012 (2022) |
| Popis: | MISTRAL is a millimetric camera working in the W-band (78–103 GHz) which will take data from the Sardinia Radio Telescope, the Italian 64-m radio telescope located 50 km form Cagliari, at 600m above the sea level, in Sardinia. It is being built as a facility instrument by the Sapienza University for INAF, that manages the radio telescope, under a PON contract. It will consist of a compact cryostat hosting the re–imaging optics, cooled at 4K, and a 408–pixel array of photon–noise limited lumped element kinetic inductance detectors fabricated at CNR-IFN and cooled at a base temperature lower than 300mK. MISTRAL will be able to investigate a long list of scientific targets spanning from extragalactic astrophysics to solar system science, with high angular resolution (~ 12 arcsec), including Sunyaev Zel’dovich effect measurements and the study of the Cosmic Web. |
| Databáze: | OpenAIRE |
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